On the Juno radio science experiment: models, algorithms and sensitivity analysis. Issue 3 (2nd December 2014)

• Record Type: Journal Article
• Authors: Tommei, G.; Dimare, L.; Serra, D.; Milani, A.
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 446:Issue 3(2015)
• Page Start: 3089
• Page End: 3099
• Publication Date: 2014-12-02
• Subjects: methods: numerical -- space vehicles -- planets and satellites: individual: Jupiter; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stu2328
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: Juno is a NASA mission launched in 2011 with the goal of studying Jupiter. The probe will arrive to the planet in 2016 and will be placed for one year in a polar high-eccentric orbit to study the composition of the planet, the gravity and the magnetic field. The Italian Space Agency (ASI) provided the radio science instrument KaT (Ka-Band Translator) used for the gravity experiment, which has the goal of studying the Jupiter's deep structure by mapping the planet's gravity: such instrument takes advantage of synergies with a similar tool in development for BepiColombo, the ESA cornerstone mission to Mercury. The Celestial Mechanics Group of the University of Pisa, being part of the Juno Italian team, is developing an orbit determination and parameters estimation software for processing the real data independently from NASA software odp . This paper has a twofold goal: first, to tell about the development of this software highlighting the models used, secondly, to perform a sensitivity analysis on the parameters of interest to the mission.